1 code implementation • 27 Aug 2019 • Collin D. Capano, Ingo Tews, Stephanie M. Brown, Ben Margalit, Soumi De, Sumit Kumar, Duncan A. Brown, Badri Krishnan, Sanjay Reddy
The properties of neutron stars are determined by the nature of the matter that they contain.
High Energy Astrophysical Phenomena General Relativity and Quantum Cosmology High Energy Physics - Phenomenology Nuclear Theory
1 code implementation • 5 Nov 2018 • Alexander H. Nitz, Collin Capano, Alex B. Nielsen, Steven Reyes, Rebecca White, Duncan A. Brown, Badri Krishnan
The three most significant signals in our catalog correspond to the binary black hole mergers GW150914, GW151226, and LVT151012.
General Relativity and Quantum Cosmology High Energy Astrophysical Phenomena
no code implementations • 18 Dec 2017 • Grant David Meadors, Badri Krishnan, Maria Alessandra Papa, John T. Whelan, Yuanhao Zhang
The speed could be reinvested into longer integration with a forecast sensitivity gain, 20 to 125 Hz median, of approximately 51%, or from 20 to 250 Hz, 11%, given the same per-band cost and setup.
Instrumentation and Methods for Astrophysics General Relativity and Quantum Cosmology
